Core-scale magnetic fields inferred using high-resolution and sensitive dust emission polarization observations using JCMT. (IMAGE)

Chinese Academy of Sciences Headquarters

Core-scale magnetic fields inferred using high-resolution and sensitive dust emission polarization observations using JCMT.

Caption

Core-scale magnetic fields (red segments) inferred using high-resolution and sensitive dust emission polarization observations using JCMT. The Solar-type star forming cores fragmented out of B213 filament are shown.

Credit

Eswaraiah Chakali, et al. 2021

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